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dc.contributor.authorMaldacena, Juan
dc.contributor.authorStrominger, Andrew
dc.date.accessioned2019-09-27T13:19:13Z
dc.date.issued1998
dc.identifier.citationMaldacena, Juan, and Andrew Strominger. 1998. “Statistical Entropy of de Sitter Space.” Journal of High Energy Physics 1998 (2): 014–014. https://doi.org/10.1088/1126-6708/1998/02/014.
dc.identifier.issn1029-8479
dc.identifier.issn1126-6708
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:41417391*
dc.description.abstractQuantum gravity in 2+1 dimensions with a positive cosmological constant can be represented as an SL(2,C) Chern-Simons gauge theory. The symmetric vacuum of this theory is a degenerate configuration for which the gauge fields and spacetime metric vanish, while de Sitter space corresponds to a highly excited thermal state. Carlip's approach to black hole entropy can be adapted in this context to determine the statistical entropy of de Sitter space. We find that it equals one-quarter the area of the de Sitter horizon, in agreement with the semiclassical formula.
dc.language.isoen_US
dc.publisherSpringer Verlag
dash.licenseLAA
dc.titleStatistical entropy of de Sitter space
dc.typeJournal Article
dc.description.versionVersion of Record
dc.relation.journalJournal of High Energy Physics
dash.depositing.authorStrominger, Andrew E.::1691de051847e2356acbdc1ec81c7333::600
dc.date.available2019-09-27T13:19:13Z
dash.workflow.comments1Science Serial ID 47380
dc.identifier.doi10.1088/1126-6708/1998/02/014
dash.source.volume1998;2
dash.source.page14-14


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